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Stars and Galaxies. Types of Stars. Color: Cooler stars are red. As they get hotter they turn orange, yellow and then blue. Composition Stars are made of different forms of gases Inner layers are dense and hot Outer layers are made up of cool gases. Brightness Brightest stars:
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Color: • Cooler stars are red. As they get hotter they turn orange, yellow and then blue. • Composition • Stars are made of different forms of gases • Inner layers are dense and hot • Outer layers are made up of cool gases
Brightness • Brightest stars: called first-magnitude stars • Dimmest stars: called sixth-magnitude stars • Positive numbers represent dimmest starts • Negative numbers represent brighter stars • Sirius (Dog star) has a magnitude of -1.4
Motion of stars: • Because of the Earth’s motion stars appear to rotate around Polaris (North star) • However, stars are moving in space, but it can take thousands of years to see the movement
First stage: • enters its life cycle as a ball of gas and dust • Life Cycle of Stars • Gravity pulls the gas and dust together into a sphere • Sphere gets hotter and denser and the hydrogen changes to helium in a process called nuclear fusion
Second stage: • Main-sequence star • Longest stage • Energy is made as hydrogen fuses into helium • Third stage: Giants and Supergiants • Red giant: star that expands and cools because it has used all its hydrogen • Red giants can be 10x bigger than the sun • Supergiants can be 100x bigger than the sun
Fourth stage: White dwarf • small hot star that is the leftover center of an older star • Can shine for billions of years before they cool completely and the star dies
Other Star deaths • Supernova: gigantic explosion in which a large massive star collapses and throws its outer layers into space • Can form a neutron star if the center of the collapsed star contracts to form a new star • if the neutron star is spinning it is called a pulsar • Can form a Black hole if the center of the collapsed star has a mass that is more than 3 times larger than our sun • Gravity pulls so strong that even light can not escape • We can detect black holes X rays to look at nearby light spiraling into the black hole
H-R Diagram • Graph that shows the relationship between a star’s surface temperature and how bright it glows (absolute magnitude)
Galaxies • large groups of stars, dust, and gas • Edwin Hubble began to classify galaxies by shape in the 1920’s.
Types of galaxies • Spiral galaxies: • Has a bulge at the center and spiral arms • Spiral arms are made up of gas, dust, and new stars • Our galaxy, The Milky Way, is thought to be a spiral galaxy
Types of galaxies • Elliptical galaxies: • Has a very bright center and very little dust and gas • Contain mostly old stars • Irregular galaxies: • The leftovers which don’t fit into any other class
What’s in a galaxy? • Billions of stars and some planetary systems • Nebulas: large clouds of gas and dust • Usually found in spiral galaxies
Origin of galaxies • Looking at distance galaxies reveals what early galaxies looked like • Among the most distance objects we can see now are quasars • Quasars: star like sources of light that are extremely far away • A very powerful energy source • May be formed from black holes in the center of some galaxies